Microwave detection of interstellar NO

Details Microwave detection of interstellar NO Microwave detection of interstellar NO

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...224l..73l&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 224, Sept. 1, 1978, p. L73-L76.

Astronomy and Astrophysics

Astronomy

28

Abundance, Interstellar Chemistry, Interstellar Gas, Microwave Emission, Nitric Oxide, Radio Astronomy, Microwave Spectra, Thermodynamic Equilibrium

Scientific paper

The strongest hyperfine component of each of the two 2 Pi 1/2, J = 3/2 = 1/2 rotational transitions of (N-14)(O-16) at 150.2 and 150.5 GHz has been detected toward Sgr B2(OH). A column density of approximately 2 x 10 to the 16th power per sq cm and a relative abundance of the order of one hundred millionth are inferred. These results are taken to indicate that nitric oxide is a fairly abundant molecular constituent of Sgr B2(OH).

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